{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:WWQWORAXAWOW7LTZ7BCZV5OFIF","short_pith_number":"pith:WWQWORAX","schema_version":"1.0","canonical_sha256":"b5a1674417059d6fae79f8459af5c541553d22c80cdd7a32d1bd2c6f3ba84038","source":{"kind":"arxiv","id":"1305.1801","version":1},"attestation_state":"computed","paper":{"title":"The very energetic, broad-lined type Ic Supernova 2010ah (PTF10bzf) in the context of GRB/SNe","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.CO","authors_text":"2, 3), 5), 6), Alessandra Corsi (8), Avishay Gal-Yam (10) ((1) INAF-OAPadova (2) Astrophysics Research Institute, Elena Pian (5, Emma S. Walker (4, John Moores Univ. (3) MPA (4) Yale University (5) Scuola Normale Superiore di Pisa (6) INAF-IASFBO (7) NAOJ (8) George Washington Univ. (9) Subaru Telescope (10) Weizmann Institute of Science), Masaomi Tanaka (7), Paolo A. Mazzali (1, Takashi Hattori (9)","submitted_at":"2013-05-08T12:50:42Z","abstract_excerpt":"SN2010ah, a very broad-lined type Ic SN discovered by the Palomar Transient Factory, was interesting because of its relatively high luminosity and the high velocity of the absorption lines, which was comparable to that of GRB/SNe, suggesting a high explosion kinetic energy. However, no GRB was detected in association with the SN. Here, the properties of SN2010ah are determined with higher accuracy than previous studies through modelling. New Subaru telescope photometry is presented. A bolometric light curve is constructed taking advantage of the spectral similarity with SN1998bw. Radiation tra"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"1305.1801","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-05-08T12:50:42Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"130f958f5c38e67460cf39fd259336130c4b360b3214790d1d9b6d83d7502c4e","abstract_canon_sha256":"b52e07a1bbb7491e386be9207b23f993e7f10cadabced88ba72644153c38f2a2"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:50:04.769470Z","signature_b64":"7qW+Hn/hdKo8rJyNmZ1aIjVFws8NlXqzPGyh8z6N56218i0B1rWDR++d4nDBZxfFfBRawvUlcSb1JYTAVSraAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b5a1674417059d6fae79f8459af5c541553d22c80cdd7a32d1bd2c6f3ba84038","last_reissued_at":"2026-05-18T01:50:04.768883Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:50:04.768883Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The very energetic, broad-lined type Ic Supernova 2010ah (PTF10bzf) in the context of GRB/SNe","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.CO","authors_text":"2, 3), 5), 6), Alessandra Corsi (8), Avishay Gal-Yam (10) ((1) INAF-OAPadova (2) Astrophysics Research Institute, Elena Pian (5, Emma S. Walker (4, John Moores Univ. (3) MPA (4) Yale University (5) Scuola Normale Superiore di Pisa (6) INAF-IASFBO (7) NAOJ (8) George Washington Univ. (9) Subaru Telescope (10) Weizmann Institute of Science), Masaomi Tanaka (7), Paolo A. Mazzali (1, Takashi Hattori (9)","submitted_at":"2013-05-08T12:50:42Z","abstract_excerpt":"SN2010ah, a very broad-lined type Ic SN discovered by the Palomar Transient Factory, was interesting because of its relatively high luminosity and the high velocity of the absorption lines, which was comparable to that of GRB/SNe, suggesting a high explosion kinetic energy. However, no GRB was detected in association with the SN. Here, the properties of SN2010ah are determined with higher accuracy than previous studies through modelling. New Subaru telescope photometry is presented. A bolometric light curve is constructed taking advantage of the spectral similarity with SN1998bw. Radiation tra"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1305.1801","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"1305.1801","created_at":"2026-05-18T01:50:04.768949+00:00"},{"alias_kind":"arxiv_version","alias_value":"1305.1801v1","created_at":"2026-05-18T01:50:04.768949+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1305.1801","created_at":"2026-05-18T01:50:04.768949+00:00"},{"alias_kind":"pith_short_12","alias_value":"WWQWORAXAWOW","created_at":"2026-05-18T12:28:06.772260+00:00"},{"alias_kind":"pith_short_16","alias_value":"WWQWORAXAWOW7LTZ","created_at":"2026-05-18T12:28:06.772260+00:00"},{"alias_kind":"pith_short_8","alias_value":"WWQWORAX","created_at":"2026-05-18T12:28:06.772260+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/WWQWORAXAWOW7LTZ7BCZV5OFIF","json":"https://pith.science/pith/WWQWORAXAWOW7LTZ7BCZV5OFIF.json","graph_json":"https://pith.science/api/pith-number/WWQWORAXAWOW7LTZ7BCZV5OFIF/graph.json","events_json":"https://pith.science/api/pith-number/WWQWORAXAWOW7LTZ7BCZV5OFIF/events.json","paper":"https://pith.science/paper/WWQWORAX"},"agent_actions":{"view_html":"https://pith.science/pith/WWQWORAXAWOW7LTZ7BCZV5OFIF","download_json":"https://pith.science/pith/WWQWORAXAWOW7LTZ7BCZV5OFIF.json","view_paper":"https://pith.science/paper/WWQWORAX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1305.1801&json=true","fetch_graph":"https://pith.science/api/pith-number/WWQWORAXAWOW7LTZ7BCZV5OFIF/graph.json","fetch_events":"https://pith.science/api/pith-number/WWQWORAXAWOW7LTZ7BCZV5OFIF/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/WWQWORAXAWOW7LTZ7BCZV5OFIF/action/timestamp_anchor","attest_storage":"https://pith.science/pith/WWQWORAXAWOW7LTZ7BCZV5OFIF/action/storage_attestation","attest_author":"https://pith.science/pith/WWQWORAXAWOW7LTZ7BCZV5OFIF/action/author_attestation","sign_citation":"https://pith.science/pith/WWQWORAXAWOW7LTZ7BCZV5OFIF/action/citation_signature","submit_replication":"https://pith.science/pith/WWQWORAXAWOW7LTZ7BCZV5OFIF/action/replication_record"}},"created_at":"2026-05-18T01:50:04.768949+00:00","updated_at":"2026-05-18T01:50:04.768949+00:00"}